A method to remove residual OH emission from near-infrared spectra

By Roger Davies. 2007

167 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Spectroscopy

View Paper: https://www.semanticscholar.org/paper/804ea5ff870acb13bdeeb4406cd56623e0ab8c1c

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In Astronomy and Astrophysics

1. P. Hopkins
2. L. Hernquist
3. D. M. Alexander
4. A. Dekel
5. R. Somerville
6. Thomas J. Cox
7. R. Dav'e
8. T. Naab

In Spectroscopy

1. S. Chapman
2. S. Lilly
3. R. Genzel
4. L. Tacconi
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6. E. Hicks
7. R. Bacon
8. J. Richard

Citations in the corpus

• THE DATA REDUCTION PIPELINE FOR THE SDSS-IV MaNGA IFU GALAXY SURVEY (2016, methodology): “This is partially because a similar degree of freedom is introduced by the 2d polyno- mial, and partially because OH features can vary in strength independently from the underlying continuum background (see, e.g., Davies 2007).”
• THE SINS SURVEY OF z ∼ 2 GALAXY KINEMATICS: PROPERTIES OF THE GIANT STAR-FORMING CLUMPS (2010, methodology): “For a description of the data reduction methods and analysis tools we refer to Schreiber et al. (2004), Davies (2007), and Förster Schreiber et al. (2009).”
• THE BLACK HOLE MASS IN M87 FROM GEMINI/NIFS ADAPTIVE OPTICS OBSERVATIONS (2011, background): “There are techniquesto bundle atmospheric emission lines into common transition families and fit a series of scalings between science and sky frames to minimize the residuals (Oliva & Origlia 1992, Rousselot et al. 2000, Davies 2007), but we have not employed them here.”
• Inferences on the timeline of reionization at z ∼ 8 from the KMOS Lens-Amplified Spectroscopic Survey (2019, methodology): “We run the pipeline including optimised sky subtraction routines sky_tweak (Davies 2007) and sky_scale.”
• ZAP -- Enhanced PCA Sky Subtraction for Integral Field Spectroscopy (2016, methodology): “The correlation in the intensity of sky emission lines associated with vibrational bands has also been observed and used to aid in sky subtraction for spectroscopy in the near infrared (Davies 2007).”
• A Close Look at Star Formation around Active Galactic Nuclei (2007, methodology): “PSF Estimation There are a multitude of ways to derive the point-spread function (PSF) from AO data, five of which are described in Davies (2007b).”
• LSD: Lyman-break galaxies Stellar populations and Dynamics – I. Mass, metallicity and gas at z∼ 3.1 (2009, methodology): “Data were reduced by using the ESO pipeline (Modigliani et al. 2007) with the improved sky subtraction described by Davies (2007).”
• THE SINS/zC-SINF SURVEY of z ∼ 2 GALAXY KINEMATICS: OUTFLOW PROPERTIES (2012, methodology): “…(∼ 6h average integration time per galaxy, with a range from 2 to 22h, and a total integration time for the entire sample of 180h) and were reduced with our standard data reduction methods and analysis tools (Schreiber et al. 2004; Davies 2007; Förster Schreiber et al. 2009; Mancini et al. 2011).”
• THE LICK AGN MONITORING PROJECT: THE MBH–σ* RELATION FOR REVERBERATION-MAPPED ACTIVE GALAXIES (2010, methodology): “The OSIRIS pipeline includes an implementation of the scaled skysubtraction algorithm described by Davies (2007), which provides a more accurate subtraction of the strong Hband airglow lines than a direct subtraction of the offsetsky exposure.”
• An atmospheric radiation model for Cerro Paranal - I. The optical spectral range (2012, background): “Data calibration and reduction also benefit from a good knowledge of atmospheric eff cts (see e.g. Davies 2007).”
• Energetic galaxy-wide outflows in high-redshift ultraluminous infrared galaxies hosting AGN activity (2012, methodology): “Attempts to remove residual OH sky emission lines wre made using the sky-subtraction techniques described in Davies (2007).”